Newtonian world and astrophysics: Ideal gases Flashcards

1
Q

how many particles are there in a mole and what is it known as

A

6.02x10^23, Avogadro’s constant

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2
Q

what are the 5 assumptions of ideal gas behaviour

A

The gas contains a very large number of atoms or molecules moving in random directions with random speeds

The atoms or molecules of the gay occupy a negligible volume compared with the volume of the gas

The collisions of atoms or molecules with each other and the container walls are perfectly elastic
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The time of collisions between the atoms or molecules is negligible compared to the time between collisions

Electrostatic forces between atoms or molecules are negligible except during collisions

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3
Q

describe the proportion between pressure and volume for an ideal gad

A

p∝1/V

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4
Q

Describe the proportion between pressure and temperature for an ideal gas

A

p∝T

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5
Q

What is the equation of an ideal gas

A

pV=nRT where n is the number of moles and R is the molar gas constant

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6
Q

what is the alternate way to write the ideal gas equation pV=nRT

A

pV=NkT where N is the number of particles and k is the Boltzmann constant

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7
Q

how do you find the r.m.s speed for a known sample

A

square the speeds, take the mean and root the answer

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8
Q

what equation links volume and m.s speed

A

pV=1/3 Nm(mean squared speed)

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9
Q

as the temperature of a gas increases what happens to the distribution of the speeds of the particle

A

the most probable speed increases and gets wider however the number of particles with a speed v reduces as there is a wider spread of speeds

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10
Q

what is the Boltzmann constant defined as

A

molar gas constant/ Avogadro constant

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11
Q

what 2 equations do you use to link kinetic energy to temperature

A

pV=1/3Nm(mean quared speed)

pV=NkT

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12
Q

if atoms of different mass have the same kinetic energy, how does speed vary

A

the heavier atoms have a lower speed

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13
Q

define internal energy

A

the sum of the kinetic and potential energies of the particles inside the gas

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